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NASA, (2010). Star Child Question of the Month for April 2001. Accessed on 15/9/5015 from
http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question32.html
Question:
What is the orbital period of the Moon?
Answer:
There are two periods involved with the orbit of the Moon around the Earth. This often leads
to some confusion, but can be easily understood. Let's investigate!
Sidereal Period versus Synodic Period

Measuring the motion of the Moon around the Earth relative to the distant stars leads
us to what is called the sidereal period. The sidereal period is the time required for a
celestial body within our solar system to complete one revolution with respect to the
fixed stars‹i.e., as observed from some fixed point outside the system. The sidereal
period of the Moon is the time needed for it to return to the same position against the
background of stars.
The Moon appears to move completely around the celestial sphere once in about 27.3
days as observed from the Earth. This is called a sidereal month. It represents the
orbital period of the Moon around the Earth.

Measuring the motion of the Moon around the Earth relative to the Sun leads us to
what is called the synodic (pronounced si-nod-ik) period. The synodic period is the
time required for a body within the solar system, such as a planet, the Moon, or an
artificial Earth satellite, to return to the same or approximately the same position
relative to the Sun as seen by an observer on the Earth. The Moon's synodic period is
the time between successive recurrences of the same phase; e.g., between full moon
and full moon.
The Moon takes 29.5 days to return to the same point on the celestial sphere as
referenced to the Sun because of the motion of the Earth around the Sun; this is called
a synodic month (lunar phases as observed from the Earth are correlated with the
synodic month).
So why are the sidereal and synodic lunar months not equal in length?
Remember that the Earth moves in its own orbit around the Sun. The synodic period is
related to the lunar phases; it depends on the relative locations of the Sun-Earth-Moon. If we
start measuring at Full Moon, then one sidereal month later we will not yet be back to a Full
Moon, since the Moon must travel further in its orbit around the Earth to reach the same
relative Sun-Earth-Moon alignment...all because during the 27.3 days of the sidereal month,
the Earth moved along in its orbit around the Sun and now the Moon must "catch up" to this
new position. It takes it just over 2 days to do so.